Multi-wavelength emission from massive star associations

Details Multi-wavelength emission from massive star associations Multi-wavelength emission from massive star associations

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459...37c&link_type=abstract

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:

Physics

Stars: Early-Type, Supernovae: General, Open Clusters And Associations: General

Scientific paper

Results from a new multi-wavelength evolutionary synthesis model including the γ-ray line emission from various radioactive isotopes (26Al, 60Fe) are presented. In particular the predicted γ-ray line observations combined with measurements of ionising fluxes can efficiently constrain the age of a stellar population, and help to identify the primary nucleosynthesis sources of the radioisotopes.

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